Published January 1, 2010
| Version v1
Conference paper
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Towards the Equation of State for Dense Stellar Matter
- 1. Selcuk Univ, Dept Phys, TR-42079 Konya, Turkey
- 2. Russian Acad Sci, Inst Nucl Res, Y Moscow 117312, Russia
Description
The thermal nuclear multifragmentation reaction can be used to investigate the nuclear liquid-gas phase coexistence region and its relation to the astrophysical processes such as the collapse of massive stars, and the supernova type-II explosions. We have performed some calculations to estimate stellar equation of state (EOS) on the basis of statistical multifragmentation model.
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